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3° Radionet Engineering Forum Workshop: Cryogenic Low Noise Components - June 19, 2006 Onsala Space Observatory, Gothenburg, Sweden
NATIONAL INSTITUTE for ASTROPHYSICS - RADIOASTRONOMY
I N A F
Cryogenic Low Noise Amplifiers from 4 Ghz up to 100 GHz
A. Cremonini1 , W.Ciccognani2, S. Mariotti1, A.Orfei1, J.Roda1, G.Tofani1
1 INAF – Institute of Radioastronomy- Bologna – Italy2 University “Tor Vergata” – Electronic Eng. Dept. – Rome - Italy
3° Radionet Engineering Forum Workshop: Cryogenic Low Noise Components - June 19, 2006 Onsala Space Observatory, Gothenburg, Sweden
NATIONAL INSTITUTE for ASTROPHYSICS - RADIOASTRONOMY
I N A F
Overview
• LNA Realisation process• MMIC design• 22GHZ LNA Characterisation• From 4 to 15 Ghz LNA design and first step measurements• Conclusion
3° Radionet Engineering Forum Workshop: Cryogenic Low Noise Components - June 19, 2006 Onsala Space Observatory, Gothenburg, Sweden
NATIONAL INSTITUTE for ASTROPHYSICS - RADIOASTRONOMY
I N A FRealization process
SpecifiesDefinition
Electrical design
Mechanical design
Packaging
Measurement
Goal: Design in order to minimize the steps back.
3° Radionet Engineering Forum Workshop: Cryogenic Low Noise Components - June 19, 2006 Onsala Space Observatory, Gothenburg, Sweden
NATIONAL INSTITUTE for ASTROPHYSICS - RADIOASTRONOMY
I N A F
Aims : Custom LNA’sThe “best” for noiseCryogenicHigh performances yield
Key technology : InP 0,1um NGC MMIC Process: 2Wafer runs
Design Tools : Foundry models @ 290K HEMT noise modeled @ 60% Idss for LIBRA IVUnknown Frequency rangeCSIRO Layout Tools based on Foundry manualEM Simulator for complex situations
Design Methodology : Design @ 290K, with separate biasingDesign “As Simple as possible”MMIC topology reviewCross checking design
3° Radionet Engineering Forum Workshop: Cryogenic Low Noise Components - June 19, 2006 Onsala Space Observatory, Gothenburg, Sweden
NATIONAL INSTITUTE for ASTROPHYSICS - RADIOASTRONOMY
I N A F
22 GHz InP MMIC
EDA Software provided by the Roma Tor Vergata UniversityEntirely designed and realized by INAFMedicina Labs Measured
3,2 mm
2,25 mm
44 mm
3° Radionet Engineering Forum Workshop: Cryogenic Low Noise Components - June 19, 2006 Onsala Space Observatory, Gothenburg, Sweden
NATIONAL INSTITUTE for ASTROPHYSICS - RADIOASTRONOMY
I N A F
Monomaterial Package•Silvar K Carrier and Chip attached with H20E
• Si30/Al70 Carrier and Chip attached with H20E
Amplifier Packaging
Bimaterial Package (main carrier : Brass)• Silvar K Island and Chip attached with H20E
• Si30/Al70 Island and Chip attached with H20E
H20E is a commercial conductive epoxy
3° Radionet Engineering Forum Workshop: Cryogenic Low Noise Components - June 19, 2006 Onsala Space Observatory, Gothenburg, Sweden
NATIONAL INSTITUTE for ASTROPHYSICS - RADIOASTRONOMY
I N A F
4245 020 22LNA_05A
Input Return Loss
Better than-16 dB over 50% BW
INSTITUTE OF RADIOASTRONOMY
Spar On Wafer Measurements
18 20 22 24 26Frequency (GHz)
4245 020 LNA_05A S11
-40
-30
-20
-10
0
Measured
Simulated
Packaged
5 15 25 35Frequency (GHz)
4245 020 LNA_05A S21
0
10
20
30
40
Measured
Simulated
Packaged
18 26Frequency (GHz)
4245 020 LNA_05A S22
-30
-20
-10
0
SimulatedPackaged
Measured
Output Return Loss
Better than-16 dB over 50% BW
Gain
(29 ± 0,5 ) dB On the whole BW
3° Radionet Engineering Forum Workshop: Cryogenic Low Noise Components - June 19, 2006 Onsala Space Observatory, Gothenburg, Sweden
NATIONAL INSTITUTE for ASTROPHYSICS - RADIOASTRONOMY
I N A F22 GHz InP MMICNoise @ 290 K on chip First order meas. accuracy ± 0.2 dB
Noise source On and Off stage Matcing IMPROVED
Noise source ENR Table Re-characterisation
High accuracy meas. ± 0.06 dB
Noise Performances 4245-020 22LNA_05A
60
100
140
180
220
260
15,5
16,5
17,5
18,5
19,5
20,5
21,5
22,5
23,5
24,5
25,5
26,5
Frequency [GHz]
T e [K
]
050201 Simulated
Noise Performances 4245-020 22LNA_05A
60
100
140
180
220
260
15,5
16,5
17,5
18,5
19,5
20,5
21,5
22,5
23,5
24,5
25,5
26,5
Frequency [GHz]
T e [K
]
050201 050201 High Accuracy Simulated
3° Radionet Engineering Forum Workshop: Cryogenic Low Noise Components - June 19, 2006 Onsala Space Observatory, Gothenburg, Sweden
NATIONAL INSTITUTE for ASTROPHYSICS - RADIOASTRONOMY
I N A F
Te Statistical distribution @ 22 GHzmeasured on wafer
100 devices distributed
over 5 wafer
14K spread @ ± 2 σ
3° Radionet Engineering Forum Workshop: Cryogenic Low Noise Components - June 19, 2006 Onsala Space Observatory, Gothenburg, Sweden
NATIONAL INSTITUTE for ASTROPHYSICS - RADIOASTRONOMY
I N A F
22 GHz InP MMIC @ 290 K (packaged)
3° Radionet Engineering Forum Workshop: Cryogenic Low Noise Components - June 19, 2006 Onsala Space Observatory, Gothenburg, Sweden
NATIONAL INSTITUTE for ASTROPHYSICS - RADIOASTRONOMY
I N A F
22 GHz InP MMIC @ 20 K ( Packaged )
3° Radionet Engineering Forum Workshop: Cryogenic Low Noise Components - June 19, 2006 Onsala Space Observatory, Gothenburg, Sweden
NATIONAL INSTITUTE for ASTROPHYSICS - RADIOASTRONOMY
I N A F
X Giornata di Studio Sull’Ingegneria Delle Microonde: SRT, RICERCHE E SVILUPPI DELLA STRUMENTAZIONE: CRYO LNA
Gain FluctuationNegligible gain fluctuations up to 1000 sec integration.
3° Radionet Engineering Forum Workshop: Cryogenic Low Noise Components - June 19, 2006 Onsala Space Observatory, Gothenburg, Sweden
NATIONAL INSTITUTE for ASTROPHYSICS - RADIOASTRONOMY
I N A F
Second run LNA specifications
10040015MMIC InP90 - 1156028017MMIC InP70 - 903515527MMIC InP33 - 502513525MMIC InP26 - 402012523MMIC InP26 - 4033535MIC & MMIC4 - 8
Te @ 20 [K] (estimated)
Te @ 290 [K]
Gain [dB] (Typical)
TechnologyFrequencyRange [GHz]
3° Radionet Engineering Forum Workshop: Cryogenic Low Noise Components - June 19, 2006 Onsala Space Observatory, Gothenburg, Sweden
NATIONAL INSTITUTE for ASTROPHYSICS - RADIOASTRONOMY
I N A F
Designed By Mecsa for Pharos Project
External Input matching Network
3 stages
3,2 x 2,5 mm
RFIN
VD1
VG2
VD3
RFOUT
VD2
VG3
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
1 1.5 2 2.5 3 3.5 4 4.5 5 5.5 6 6.5 7 7.5 8 8.5 9 9.5 10Frequency (GHz)
6LNA_01A Spar
-80-75-70-65-60-55-50-45-40-35-30-25-20-15-10-505
1015202530354045
-40-35-30-25-20-15-10-50510152025303540455055606570758085
4 - 8 GHz InP MMIC LNA
1 1.5 2 2.5 3 3.5 4 4.5 5 5.5 6 6.5 7 7.5 8 8.5 9 9.5 10Frequency (GHz)
6LNA_01A Spar
-80-75-70-65-60-55-50-45-40-35-30-25-20-15-10-505
1015202530354045
-40-35-30-25-20-15-10-50510152025303540455055606570758085
1 1.5 2 2.5 3 3.5 4 4.5 5 5.5 6 6.5 7 7.5 8 8.5 9 9.5 10Frequency (GHz)
6LNA_01A Spar
-80-75-70-65-60-55-50-45-40-35-30-25-20-15-10-505
1015202530354045
-40-35-30-25-20-15-10-50510152025303540455055606570758085
1 1.5 2 2.5 3 3.5 4 4.5 5 5.5 6 6.5 7 7.5 8 8.5 9 9.5 10Frequency (GHz)
6LNA_01A Spar
-80-75-70-65-60-55-50-45-40-35-30-25-20-15-10-505
1015202530354045
-40-35-30-25-20-15-10-50510152025303540455055606570758085
S21
S11
S22
6LNA_01A
0,00
20,00
40,00
60,00
80,00
100,00
120,00
140,00
160,00
180,00
200,00
4 4,5 5 5,5 6 6,5 7 7,5 8
Fre q [GHz]
Te
[K
MMIC Simulation
Off Chip Match Net
MMIC MeasureMMIC SimulationMMIC Measure
Off Chip Match Net
3° Radionet Engineering Forum Workshop: Cryogenic Low Noise Components - June 19, 2006 Onsala Space Observatory, Gothenburg, Sweden
NATIONAL INSTITUTE for ASTROPHYSICS - RADIOASTRONOMY
I N A F
3,2 x 2,25 mm
20 22 24 26 28 30 32 34 36 38 40 42 44 46 48 50Frequency (GHz)
32LNA_01A Spar
-25-20-15-10-505
101520253035404550556065707580
-65-60-55-50-45-40-35-30-25-20-15-10-50510152025303540
VG 2 VG 4
RFO UT
VD3VD2
VG 3
VD1
VG 1
RFI N
VD4
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
26 - 40 GHz InP MMIC LNA – 1° Version
4 stages snake shapeGain >30 dBIRL < -12 dBORL < -15
S21
S11S22
32LNA_01A
100
110
120
130
140
150
160
170
180
190
200
210
26 27 28 29 30 31 32 33 34 35 36 37 38 39
Freq [GHz]
Te [K
]
3° Radionet Engineering Forum Workshop: Cryogenic Low Noise Components - June 19, 2006 Onsala Space Observatory, Gothenburg, Sweden
NATIONAL INSTITUTE for ASTROPHYSICS - RADIOASTRONOMY
I N A F
3,2 x 2,25 mm
RFOUT
VG2
VD3VD1
VD2
VG3
RFIN
VG1
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
20 22 24 26 28 30 32 34 36 38 40 42 44 46 48 50Frequency (GHz)
32LNA_02A Spar
-65
-55
-45
-35
-25
-15
-5
5
15
25
35
-30
-20
-10
0
10
20
30
40
50
60
70
26 - 40 GHz InP MMIC LNA 2° Version
3 stagesGain >25 dBIRL < -15 dBORL < -10
S21
S11
S22
32LNA_02A
100,00110,00120,00130,00140,00150,00160,00170,00180,00190,00200,00210,00220,00230,00240,00250,00
26 27 28 29 30 31 32 33 34 35 36 37 38 39
Freq [GHz]
Te [K
]
3° Radionet Engineering Forum Workshop: Cryogenic Low Noise Components - June 19, 2006 Onsala Space Observatory, Gothenburg, Sweden
NATIONAL INSTITUTE for ASTROPHYSICS - RADIOASTRONOMY
I N A F
3,2 x 2,25 mm
VG 1
VD3
VG4VG3
VD2
RFI N
VG2
VD1VD4
RFOUT
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
33 - 50 GHz InP MMIC LNA
20 22 24 26 28 30 32 34 36 38 40 42 44 46 48 50Frequency (GHz)
43LNA_01A Spar
-30-25-20-15-10
-505
101520253035404550556065707580
-70-65-60-55-50-45-40-35-30-25-20-15-10-50510152025303540
4 stagesGain >32 dBIRL < -15 dBORL < -10
S21
S11
S22
43L NA_01A
100 ,00110 ,00120 ,00130 ,00140 ,00150 ,00160 ,00170 ,00180 ,00190 ,00200 ,00210 ,00220 ,00230 ,00240 ,00250 ,00260 ,00270 ,00280 ,00290 ,00300 ,00310 ,00320 ,00330 ,00340 ,00350 ,00
33 35 37 39 41 43 45 47 49
F req [G Hz]
Te [K
3° Radionet Engineering Forum Workshop: Cryogenic Low Noise Components - June 19, 2006 Onsala Space Observatory, Gothenburg, Sweden
NATIONAL INSTITUTE for ASTROPHYSICS - RADIOASTRONOMY
I N A F
3,2 x 2,25 mm
RFO UT
VG 3
VD3
VG1
VD1
VG4
RFI N
VD4
VG2
VD2
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
70 - 90 GHz InP MMIC LNA
70 72 74 76 78 80 82 84 86 88 90 92 94 96 98 100Frequency (GHz)
86LNA_01A Spar
-70-65-60-55-50-45-40-35-30-25-20-15-10
-505
10152025
-35-30-25-20-15-10-5051015202530354045505560
4 stagesGain >15 dBIRL < -10 dBORL < -15
S21
S11
S22
86LNA_01A
100,00
150,00
200,00
250,00
300,00
350,00
400,00
450,00
500,00
550,00
600,00
72 73 74 75 76 77 78 79 80 81 82 83 84 85 86 87 88 89 90
Freq [GHz]
Te [K
]
3° Radionet Engineering Forum Workshop: Cryogenic Low Noise Components - June 19, 2006 Onsala Space Observatory, Gothenburg, Sweden
NATIONAL INSTITUTE for ASTROPHYSICS - RADIOASTRONOMY
I N A F
2,5 x 2,5 mm
RFI N
VD4
VG 3
VD1 VD3
VG1
VD2
VG2
RFOUT
VG4
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
GND:
90 - 115 GHz InP MMIC LNA
80 82 84 86 88 90 92 94 96 98 100102104106108110112114116118Frequency (GHz)
100LNA_01A Spar
-80-75-70-65-60-55-50-45-40-35-30-25-20-15-10-505
10152025
-30-25-20-15-10-5051015202530354045505560657075
4 stagesGain >10 dB
S21
S11S22
100LNA_01A
100,00
150,00
200,00
250,00
300,00
350,00
400,00
450,00
500,00
550,00
600,00
90 91 92 93 94 95 96 97 98 99 100
Freq [GHz]
Te [K
]
3° Radionet Engineering Forum Workshop: Cryogenic Low Noise Components - June 19, 2006 Onsala Space Observatory, Gothenburg, Sweden
NATIONAL INSTITUTE for ASTROPHYSICS - RADIOASTRONOMY
I N A F
2001 10 100Frequency (GHz)
Gain and Noise Temperature
-10
-5
0
5
10
15
20
25
30
35
40[d
B]
0
100
200
300
400
500
600
700
800
900
1000
[K]
Frequency coverage
Te
Gain
3° Radionet Engineering Forum Workshop: Cryogenic Low Noise Components - June 19, 2006 Onsala Space Observatory, Gothenburg, Sweden
NATIONAL INSTITUTE for ASTROPHYSICS - RADIOASTRONOMY
I N A F
Conclusion….
LNA’s from 4 to 115 GHz has been designed and measured
Future….
Improve measurement accuracyPerform reverse engineeringValidate Hi freq modelValidate Cryogenic model
3° Radionet Engineering Forum Workshop: Cryogenic Low Noise Components - June 19, 2006 Onsala Space Observatory, Gothenburg, Sweden
NATIONAL INSTITUTE for ASTROPHYSICS - RADIOASTRONOMY
I N A F
CSIRO-ATNF for design, measurements support and the opportunity to approach TRW Technology
Tor Vergata University Microwave Group that shared EDA Software and skillness
European partner designers for the intense and synergic collaboration
Acknowledgements
Mecsa Facilities for Hi Accuracy noise Measurements
3° Radionet Engineering Forum Workshop: Cryogenic Low Noise Components - June 19, 2006 Onsala Space Observatory, Gothenburg, Sweden
NATIONAL INSTITUTE for ASTROPHYSICS - RADIOASTRONOMY
I N A F
Thanks